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--- tests:discs:mockub [2014/11/03 09:12] – created kawata
+++ tests:discs:mockub [2022/10/24 12:26] (current) – external edit 127.0.0.1
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+====== Barcelona Mock data Suite ======
 ===== Test particles data (Barred potential) =====
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 **The simulation data is too large to upload it to the twiki. We can provide it in a USB stick or you can find it at google drive: https://docs.google.com/file/d/0B8sgZGL4aKpSc3dlUnRKdkszaHM/edit?usp=sharing .**
+===== N-body data =====
+===Pure N-body, isolated galaxy (barred)===
+-You can find a snapshot of this model (B1), that has 1 million disk particles, at:
+Barcelona Nbody simulation 1M particles, barred model + spirals connected to the bar, centered at the Galactic Centre and bar pattern speed of 37-38 km/s/kpc. {{:tests:discs:isol_b1_stars_centered.dat.gz|}}
+http://www.am.ub.edu/~sroca/Nbody/snapshots/B1/isol_B1_stars_x8.5kpc.out (the center is at a solar position, the sun is placed in the x axis at 8.5 kpc from the galactic center)
+-In each row you will find:
+x(kpc),y(kpc),z(kpc),vx(km/s),vy(km/s),vz(km/s),mass (Msun)
+-If the user needs more snapshots from this simulation please do not hesitate to contact with Santi Roca-Fabrega (sroca@am.ub.es).
+-If using this simulation for a publication please use the following references: Roca-Fabrega et al 2013 (2013MNRAS.432.2878R) and Roca-Fabrega et al. 2014 (2014MNRAS.440.1950R)
+--Pure N-body, isolated galaxy (unbarred)--
+-You can find a snapshot of this model (U1), that has 1 million disk particles, at:
+http://www.am.ub.edu/~sroca/Nbody/snapshots/U1/isol_U1_stars_centered.out (centered to the galactic center)
+http://www.am.ub.edu/~sroca/Nbody/snapshots/U1/isol_U1_stars_x8.5kpc.out (the center is at a solar position, the sun is placed in the x axis at 8.5 kpc from the galactic center)
+-In each row you will find:
+x(kpc),y(kpc),z(kpc),vx(km/s),vy(km/s),vz(km/s),mass (Msun)
+-If the user needs more snapshots from this simulation please do not hesitate to contact with Santi Roca-Fabrega (sroca@am.ub.es).
+-If using this simulation for a publication please use the following references: Roca-Fabrega et al 2013 (2013MNRAS.432.2878R) and Roca-Fabrega et al. 2014 (2014MNRAS.440.1950R)
+Model B1 (barred model + spirals connected to the bar, 1*10^6 disk particles)
+Barcelona Nbody simulation RC sample with Bar potential (with extinction, new error model) {{:tests:discs:simb5.gc.dat|}}
+===Cosmological N-body + hydrodynamics===
+-You can find a snapshot of the stellar component that is inside 500kpc from the center of the main galactic
+system in this simulation, at redshift 0, in:
+http://www.am.ub.edu/~sroca/Hidrosim/MW_003/RUN2.3/all_stars_z0.0_r500kpc_centered.out (centered to the galactic center)
+http://www.am.ub.edu/~sroca/Hidrosim/MW_003/RUN2.3/all_stars_z0.0_r500kpc_x8.5kpc.out (the center is at a solar position, the sun is placed in the x axis at 8.5 kpc from the galactic center)
+-In each column you can find:
+x(kpc),y(kpc),z(kpc),vx(km/s),vy(km/s),vz(km/s),mass (Msun), iron (solar), alpha/iron (solar), age(Gyrs), redshift_birth , param1, param2, vcirc (km/s, GM/r approach)
+-If the user needs more snapshots from this simulation please do not hesitate to contact with Santi Roca-Fabrega (sroca@am.ub.es).
+-If using this simulation for a publication please use the following references: Roca-Fabrega et al 2015 (2015arXiv150406261R)